Welcome & Opening

• Jochen Schieck (Austrian Academy of Sciences (AT))

Room: TU the Sky

Detector requirements for future high-energy collider experiments (HEP Systems)

• Eva Sicking (CERN)

Room: TU the Sky Particle detectors for operation at future high-energy collider experiments are designed in view of both their facilities' physics objectives and their experimental conditions, which differ substantially between lepton and hadron colliders as well as between linear and circular colliders. Example differences are background conditions and duty cycles, which for instance translate into very different requirements in terms of shielding, radiation-hardness requirements and cooling concepts. Furthermore the detector designs take into account cost and engineering constraints as well as anticipate future technology developments. An overview of the physics cases and experimental environments of the currently proposed future high-energy colliders is given, including CEPC, CLIC, FCC-ee and ILC for e+e- colliders, FCC-hh, HE-LHC and SppC for pp colliders as well as muon collider concepts. The corresponding detector design choices are discussed and challenges in the design are outlined.

Dark Matter in CCDs at Modane (DAMIC-M): a silicon detector apparatus searching for low-energy physics processes (HEP Systems)

• Steven Juhyung Lee (University of Zurich (CH))

Room: TU the Sky Dark Matter In CCDs (DAMIC) is a silicon detector apparatus used primarily for searching for low-mass dark matter using the silicon bulk of Charge-Coupled Devices (CCDs) as targets. The silicon target within each CCD is 675 µm thick and its top surface is divided into over 16 million 15 µm x 15 µm pixels. The DAMIC collaboration has installed and operated seven of these CCDs at SNOLAB, achieving a pixel readout noise of 1.6 e and a leakage current as low as 2E-22A/cm^2. The low instrumental noise of the devices allowed DAMIC at SNOLAB to perform highly sensitive searches for the scattering and absorption of light dark matter particles. A new DAMIC apparatus will be installed at Laboratoire Souterrain de Modane in a few years. The DAMIC at Modane (DAMIC-M) collaboration will be using an improved version of CCDs designed by Lawrence Berkeley National Laboratory with skipper amplifiers that use non-destructive readout with multiple-sampling, enabling the CCDs to achieve a readout noise of 0.068 e. The low readout noise, in conjunction with low leakage current of these skipper CCDs, will allow DAMIC-M to observe physics processes with collisions energies less than 10 eV. The DAMIC-M experiment will consist of an array of 50 large-area skipper CCDs with more than 36 million pixels in each CCD. The following talk will introduce the DAMIC apparatus at SNOLAB and its results as well as the capabilities and the status of the new DAMIC-M experiment.

Travel to Dinner location Room: TU the Sky

Closeout

• Gian-Franco Dalla Betta (INFN and University of Trento)

Room: TU the Sky